Deflection angle of light in an black hole with primary scalar hair geometry

IF 1.9 4区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Farzan Mushtaq, Xia Tiecheng
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引用次数: 0

Abstract

Weak gravitational lensing of the primary scalar hair black hole is proposed within this work. We can figure out the deflection angle of light by applying the Gibbons and Werner approach with a primary scalar hair black hole. To do this, we compute the Gaussian curvature and find the deflection angle of the weak field limits by applying Gauss-Bonnet theorem. Furthermore, we compute the deflection angle of light when it comes across both plasma and non-plasma field. We also study how the deflection angle behaves graphically in both cases.

具有主标度发几何形状的黑洞中的光偏转角
这项研究提出了主标量发丝黑洞的弱引力透镜。我们可以通过应用吉本斯和韦纳的方法来计算主标量发丝黑洞的光偏转角。为此,我们计算了高斯曲率,并应用高斯-波内特定理找到了弱场极限的偏转角。此外,我们还计算了光穿过等离子体和非等离子体场时的偏转角。我们还研究了偏转角在这两种情况下的图形表现。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
New Astronomy
New Astronomy 地学天文-天文与天体物理
CiteScore
4.00
自引率
10.00%
发文量
109
审稿时长
13.6 weeks
期刊介绍: New Astronomy publishes articles in all fields of astronomy and astrophysics, with a particular focus on computational astronomy: mathematical and astronomy techniques and methodology, simulations, modelling and numerical results and computational techniques in instrumentation. New Astronomy includes full length research articles and review articles. The journal covers solar, stellar, galactic and extragalactic astronomy and astrophysics. It reports on original research in all wavelength bands, ranging from radio to gamma-ray.
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